Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
10700996 | Chinese Astronomy and Astrophysics | 2005 | 7 Pages |
Abstract
Using the standard Runge-Kutta method, a global solution of the basic equations describing black hole accretion flows is derived. It is proved that transition from a standard thin disk to an advection-dominated accretion flow is realizable in case of high viscosity, without introducing any additional mechanism of energy transfer or specifying any ad hoc outer boundary condition.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Lin Yi-qing, Lu Ju-fu, G.U. Wei-min,